Full text: CMRT09

In: Stilla U, Rottensteiner F, Paparoditis N (Eds) CMRT09. IAPRS, Vol. XXXVIII, Part 3/W4 — Paris, France, 3-4 September, 2009 
Figure 7: pdf of height for varying coherence (other parameters fixed). 
4. ACCURACY OF BUILDING HEIGHT ESTIMATION 
The accuracy assessment has been carried out with the scheme 
described above. Parameter values were chosen in accordance 
to the main TanDEM-X specifications. Mutual influence of 
following parameters has been investigated: 
baseline length 
incidence angle 
coherence 
amount of averaging/smoothing 
wavelength 
Figure 8 exemplifies the specific case of moderate coherence 
(0.6) and only one single look. i.e. the original spatial resolution 
is maintained and no smoothing is done. A low coherence has 
been chosen by intention, although significantly better values 
are expected for TanDEM-X, since clutter may decrease the 
coherence in layover areas. The ideal case for this configuration 
suggests to selecting a long baseline (e.g. 150m) and a steep 
incidence angle (15°), which results in a height accuracy of 
approx. 2.5m. Incidence angles less close to the system limits 
would yield an accuracy of 5m - 7m. 
The effect of improving coherence is illustrated in Figure 9, 
where height accuracy is plotted against coherence and various 
baselines. It can be seen that, for a baseline of 150m, height 
accuracy increases from 2.5m at a coherence of 0.6 up to 1.5m 
at a coherence of 0.9. 
The final assessment deals with the influence of the number of 
looks. A coherence of 0.7 for the case of 200m baseline and 15° 
incidence angle enables the derivation of building heights with 
lm accuracy for the given viewing geometry (see Figure 10). As 
this kind of averaging reduces the spatial resolution, it is 
reasonable to investigate the effect of smoothing onto the height 
accuracy only up to four looks. What is moreover evident from 
Figure 10 is that the increase of height accuracy is significant 
from one to two and three looks, but it is then gradually 
attenuating - especially for typical coherence values in the 
range of 0.6 - 0.8. 
As a last remark we refer to the used wavelength (X-band in our 
calculations). Equation 7 shows that the RADAR wavelength is 
a constant factor for the phase-to-height-sensitivity, which 
directly propagates to the standard deviation of height 
measurements. A longer wavelength (L-band for instance) 
yields a worse phase-to-height sensitivity and consequently a 
worse height accuracy. It should be noted, however, that long 
wavelengths generally yield better interferometric coherence 
depending on the scene characteristics. Hence, this effect could 
be partly compensated. 
Height Error for Correlation Coefficient = 0.6 and 1 Look 
Figure 8: Height accuracy for varying baseline and incidence angle 
while other parameters are fixed. 
Height Error for 1 Look and Incident Angle = 15® 
Figure 9: Height accuracy for varying baseline and coherence while 
other parameters are fixed. 
Figure 10: Height accuracy for varying looks and coherence while 
other parameters are fixed. 
5. DISCUSSION AND CONCLUSION 
The above analysis shows that space-borne interferometric SAR 
systems like TanDEM-X will allow to measure vertical heights 
with a standard deviation of roughly 1,5m, which also holds for 
the case of moderate coherence in layover areas. Regarding the 
application of rapid mapping, this accuracy will certainly allow 
the estimation of the number of floors or the detection of 
changes in the 3D building geometry. However, baselines and 
incidence angles have to be chosen carefully, as they are close 
to the technical limits (i.e. “critical baseline” and steep viewing 
angle). These constraints can be relaxed when additional data in 
form of digital ground plans is available. These allow, for 
instance, the utilization of specialized filters instead of simple 
multi-looking. The geometry of the filter mask can then be 
adapted to the respective building shape to include as much 
pixels as possible as observations into the height measurement. 
Recall Figure 6 to see how the standard deviation of 
interferometric phase improves with increasing number of 
observations.
	        
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